The halo of M 105 and its group environment as traced by planetary nebula populations - II. Using kinematics of single stars to unveil the presence of intragroup light around the Leo I galaxies NGC 3384 and M 105

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Fig. 6.

Modelled SB maps of NGC 3384 (left) and M 105 (centre), with the centres of the galaxies marked with red and blue crosses, respectively. Right panel: composite SB map from both galaxies and green contours where M 105 contributes 90%, 50%, and 10% of the total light distribution.

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